Data observed from 03 January, 2017 (with DA42) and from 25 December,
2016 (with DA50) until the February 2017 shutdown (31 January 2017),
and that was run through either manual or pipeline calibration and
imaging prior to 21 February, 2017, will have ...

Information about polarization in Cycle 4 can be found in the ALMA
Cycle 4 Proposer's Guide [1] section A.7.
For Cycle 4, on top of the dual polarizations (XX, YY) and single
polarization modes (XX), observations to measure the full intrinsic
pol...

NOTE: This article is only for preparation of CYCLE 4 Solar
observations.
To increase the density of the data points on the u-v plane for
obtaining high dynamic range, PIs might need to observe the Sun with
the same observing parameters twice in the...

This Knowledgebase article is a repository for information relevant to
submission of Cycle 4 proposals. These items may affect how users
write their proposals or set up their observations in the OT. The
content may evolve rapidly as the April 21, 2016 pro...

In Cycle 4, standard observing modes are those that have been used in
previous Cycles and for which the data can be reduced by the pipeline.
Please see Section 5.2 of the Cycle 4 Proposer's Guide [1].
Non-standard modes are observing modes that a...